Quark matter at finite temperature under strong magnetic fields within Nambu–Jona-Lasinio model

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成果类型：

期刊论文

作者：

Chu, Peng-Cheng*;Zhou, Yi;Chen, Chang*;Li, Xiao-Hua*;Ma, Hong-Yang*

通讯作者：

Chu, Peng-Cheng;Chen, Chang;Ma, Hong-Yang;Li, Xiao-Hua

作者机构：

[Chu, Peng-Cheng] Qingdao Technol Univ, Sch Sci, Inst Theoret Phys, Qingdao 266000, Peoples R China.

[Chu, Peng-Cheng; Chu, PC; Chen, Chang] Qingdao Technol Univ, Quantum Phys Lab, Qingdao 266000, Peoples R China.

[Zhou, Yi] Qingdao Univ Sci & Technol, Sch Math & Phys, Qingdao 266000, Peoples R China.

[Chen, Chang; Ma, Hong-Yang] Qingdao Technol Univ, Sch Sci, Qingdao 266000, Peoples R China.

[Li, Xiao-Hua] Univ South China, Sch Nucl Sci & Technol, Hengyang 421001, Peoples R China.

通讯机构：

[Chu, Peng-Cheng; Chu, PC; Chen, C; Ma, HY] Q

[Li, Xiao-Hua] U

Qingdao Technol Univ, Sch Sci, Inst Theoret Phys, Qingdao 266000, Peoples R China.

Qingdao Technol Univ, Quantum Phys Lab, Qingdao 266000, Peoples R China.

Qingdao Technol Univ, Sch Sci, Qingdao 266000, Peoples R China.

语种：

英文

关键词：

quark matter;symmetry energy;compact stars

期刊：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS

ISSN：

0954-3899

年：

2020

卷：

期：

页码：

085201

DOI：

10.1088/1361-6471/ab9b06

基金类别：

NSFCNational Natural Science Foundation of China [11975132, 11505100, 11804179, 61502262, 11205083, 41702322, 61772295]; Natural Science Foundation of Shandong, ChinaNatural Science Foundation of Shandong Province [ZR2019YQ01, ZR2019PA018, ZR2015AQ007, ZR2016DB01]; Research Foundation of Education Bureau of Hunan Province, China [15A159]; Natural Science Foundation of Hunan Province, ChinaNatural Science Foundation of Hunan Province [2015JJ3103]; Shandong Provincial Keypoint Research and Invention Program, China [2017GSF216010]

机构署名：

本校为通讯机构

院系归属：

机械工程学院

核科学技术学院

摘要：

The quark matter symmetry free energy and the thermodynamical properties of strange quark matter (SQM) in strong magnetic fields and non-zero temperature cases are discussed in this work within Nambu-Jona-Lasinio (NJL) model by considering two kinds of vector interactions. The properties of the proto-quark stars (PQSs) are also studied by introducing a density-dependent magnetic field strength distribution and assuming two 'extreme' magnetic orientation cases inside the quark stars (QSs). The results indicate that the strength and orientation d...

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Quark matter at finite temperature under strong magnetic fields within Nambu–Jona-Lasinio model

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